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	Solar activity as a consequence of the solar system origin Čech, J. ; Kotrč, Pavel ; Křivský, L. ; Klimeš, J. A similarity of the orbital periods of planets and those iccuring in the solar activity is discussed. Detailed record
	Methodology of the search of rapid changes of the H-alpha chromosphere brightness Kupryakov, Yu. A. ; Kotrč, Pavel ; Havlíčková, E. Methodology of searching fast changes in the chromosphere H-alpha brightness during solar flares is discussed. Detailed record
	Our world as an area of encounters and crossing Rajchl, Jaroslav Process of encounter and subsequent crossing leads to the formal similarity between both, the Mendelian law of meridity on the one side, and the Clifford algebra, on the other. Both representations contain a two-phase process analogical to the quantum theory paradigma and the relativistic cosmology one. Detailed record
	Spectroscopic study of omicron And Budovičová, Andrea Detailed record
	Connections and encounters, being and becoming Rajchl, Jaroslav Detailed record
	Konvence jako setkání a triáda Rajchl, Jaroslav Detailed record
	Čas a setkání. Dvakrát o dvojí podobě času či časovosti Rajchl, Jaroslav Detailed record
	O světě horizontů vědění Rajchl, Jaroslav Detailed record
	How did the last cycle of solar activity end and the new one begin Bumba, Václav ; Garcia, A. ; Klvaňa, Miroslav We demonstrate that also during the period of activity minimum on solar surface two active longitudes exist, and that active regions of both cycles closely correlate with them. We study the development of the magnetic fields in this transition phase and, above all, the influence of convection on their distribution. Detailed record
	The influence of the reference zero-velocity on the model of the vector velocity field in a symmetric sunspot Klvaňa, Miroslav ; Bumba, Václav ; Krivcovová, N. It appears that the occurrence of the vector velocity in an umbra caused by the shift of the Doppler-velocity zero-reference level can be successfully corrected by the position change of the point of symmetry of the spot. In such a case, the character of the spot vector velocity field will= be conserved. Detailed record

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